
where on the right hand side \(\omega \)  is the frequency of decay of perturbation, \(l\)  is the angular momentum of the probe scalar and \(T_{H}\)  is the blackhole temperature. Carrying forward this conjecture, an interpretation of the blackhole quasinormal modes in terms of dual thermal CFT was first suggested in [1]}. The analysis of [1]} involves numerically calculating quasinormal modes for Schwarzschild blackhole in asymptotically AdS space-time.
